Glossary term: 金星
Description: 金星是距离太阳第二近的行星,经常被称为地球的孪生兄弟。它是一颗岩石质的类地行星,半径略大于 6000 公里,约为地球半径的 95%,质量是地球质量的 0.815 倍。金星大气的密度是地球的 90 倍,它的主要成分是二氧化碳,还有浓厚的硫酸云层覆盖整个表面。厚重的大气层产生了非常强烈的温室效应,导致金星表面温度高达 460 摄氏度。
金星与太阳的平均距离为 1.08 亿公里,约为 0.72 个天文单位(日地距离)。它绕太阳公转一周需要224.7天。相较于遥远的恒星,金星绕着它的轴自转一周也需要很长时间;一个金星日相当于 243 个地球日。这比金星绕太阳运行一周的时间还要长。金星没有已知的卫星。
金星以罗马爱神维纳斯命名。由于它离太阳很近,因此在日出前或日落后的夜空中经常可以看到金星。在这种情况下,即使用肉眼观察,金星也非常明亮,传统上被称为晨星或昏星。用双筒望远镜可以看到,金星有与月亮相似的相位变化。
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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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